Triple

T11001156
Position Surface form Disambiguated ID Type / Status
Subject SARA E260006 entity
Predicate fullName P16 FINISHED
Object Sub-keV Atom Reflecting Analyzer E260006 NE FINISHED

How this triple was built (2 steps)

Every LLM step that produced this triple, in pipeline order — named-entity classification, the disambiguation choices (the exact options shown, with the pick highlighted), and the generated description. The batch + timestamp of each is in the Provenance table below.

NER Named-entity recognition gpt-5-mini
Instruction
Given a phrase, classify it is english named entity (e.g., persons, organizations, works of art) in Latin script, or not (e.g., literals, dates, URLs, verbose phrases). For disambiguation, the statement where the phrase occurs as object is also given. Please return a JSON object with `phrase` (string, the phrase being analyzed) and `is_ne` (boolean, indicating whether the phrase is a Named Entity).
Input
Phrase: Sub-keV Atom Reflecting Analyzer | Statement: [SARA, fullName, Sub-keV Atom Reflecting Analyzer]
NED1 Entity disambiguation (via context triple) gpt-5-mini-2025-08-07
Target entity: Sub-keV Atom Reflecting Analyzer
Context triple: [SARA, fullName, Sub-keV Atom Reflecting Analyzer]
  • A. SARA (Sub-keV Atom Reflecting Analyzer) chosen
    SARA (Sub-keV Atom Reflecting Analyzer) is a scientific instrument designed to study low-energy neutral atoms reflected from planetary surfaces, particularly to investigate solar wind interactions with the Moon.
  • B. Low Energy Transmission Grating Spectrometer
    The Low Energy Transmission Grating Spectrometer is a high-resolution X-ray spectrometer on the Chandra X-ray Observatory designed to disperse low-energy X-rays for detailed spectral analysis of cosmic sources.
  • C. High Energy Transmission Grating Spectrometer
    The High Energy Transmission Grating Spectrometer is a high-resolution X-ray spectrometer aboard NASA’s Chandra X-ray Observatory, designed to disperse incoming X-rays into detailed spectra for precise studies of high-energy astrophysical sources.
  • D. Photon Spectrometer
    The Photon Spectrometer is a specialized detector subsystem of the ALICE experiment at CERN designed to precisely measure and analyze high-energy photons produced in heavy-ion collisions.
  • E. Solar Isotope Spectrometer
    The Solar Isotope Spectrometer is a scientific instrument designed to precisely measure the composition and energy spectra of solar and galactic cosmic-ray isotopes.
  • F. None of above.
  • G. Unsure - the case is ambiguous/there is not enough information to decide.

Provenance (3 batches)

The batch behind each pipeline step, in order, with when it ran. Timestamps are batch-level — stages were processed in waves, so the object chain (NER → NED1 → NEDg → NED2) reads in order, but predicate / elicitation batches can sit in a different wave.

Step Stage Batch ID Status When
creating Elicitation batch_69d6aa8a6a548190a750f944ccdc8064 completed April 8, 2026, 7:20 p.m.
NER Named-entity recognition batch_69d796d68b608190a8d016b9383e82f8 completed April 9, 2026, 12:08 p.m.
NED1 Entity disambiguation (via context triple) batch_69e3453d181081908cb58a957f4d1295 completed April 18, 2026, 8:47 a.m.
Created at: April 8, 2026, 9:25 p.m.